Accretion Disk Turbulence With a Detailed Thermodynamics

Details Accretion Disk Turbulence With a Detailed Thermodynamics Accretion Disk Turbulence With a Detailed Thermodynamics

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..444...36k&link_type=abstract

5th international conference of numerical modeling of space plasma flows (astronum 2010). Proceedings of a 5th international con

Astronomy and Astrophysics

Astronomy

Scientific paper

We present recent simulations of accretion disc turbulence. These simulations include a detailed thermodynamics using radiative transfer in the one-temperature flux-limited diffusion approximation. In this paper we investigate how radiative diffusion changes the spatial structure and the turbulence for a protoplanetary accretion disc. Our simulations consider a massive protoplanetary disc model. In these models the vertical structure of the disc results from a balance of the radiative diffusion and the turbulent heating in the midplane region of the disc.

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